Relevant bibliographies by topics / High Energy Astrophysics; Cosmic Rays

Academic literature on the topic 'High Energy Astrophysics; Cosmic Rays'

Author: Grafiati
Published: 10 December 2022
Last updated: 28 January 2023

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Journal articles on the topic "High Energy Astrophysics; Cosmic Rays"

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Protheroe, R. J., and R. W. Clay. "Ultra High Energy Cosmic Rays." Publications of the Astronomical Society of Australia 21, no. 1 (2004): 1–22. http://dx.doi.org/10.1071/as03047.

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AbstractCosmic rays with energies above 1018 eV are currently of considerable interest in astrophysics and are to be further studied in a number of projects which are either currently under construction or the subject of well-developed proposals. This paper aims to discuss some of the physics of such particles in terms of current knowledge and information from particle astrophysics at other energies.
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NG, JOHNNY S. T., and PISIN CHEN. "PROSPECTS OF HIGH ENERGY LABORATORY ASTROPHYSICS." International Journal of Modern Physics B 21, no. 03n04 (February 10, 2007): 312–18. http://dx.doi.org/10.1142/s0217979207042082.

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Ultra high energy cosmic rays (UHECR) have been observed but their sources and production mechanisms are yet to be understood. We envision a laboratory astrophysics program that will contribute to the understanding of cosmic accelerators with efforts to: 1) test and calibrate UHECR observational techniques, and 2) elucidate the underlying physics of cosmic acceleration through laboratory experiments and computer simulations. Innovative experiments belonging to the first category have already been done at the SLAC FFTB. Results on air fluorescence yields from the FLASH experiment are reviewed. Proposed future accelerator facilities can provided unprecedented high-energy-densities in a regime relevant to cosmic acceleration studies and accessible in a terrestrial environment for the first time. We review recent simulation studies of non-linear plasma dynamics that could give rise to cosmic acceleration, and discuss prospects for experimental investigation of the underlying mechanisms.
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Clay, Roger W., Benjamin J. Whelan, and Philip G. Edwards. "Centaurus A at Ultra-High Energies." Publications of the Astronomical Society of Australia 27, no. 4 (2010): 439–48. http://dx.doi.org/10.1071/as09077.

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AbstractWe review the importance of Centaurus A in high-energy astrophysics as a nearby object with many of the properties expected of a major source of very high-energy cosmic rays and gamma rays. We examine observational techniques and the results so far obtained in the energy range from 200 GeV to above 100 EeV and attempt to fit those data to expectations of Centaurus Aas an astrophysical source from very high to ultra-high energies.
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WESTERHOFF, STEFAN. "ULTRA–HIGH-ENERGY COSMIC RAYS." International Journal of Modern Physics A 21, no. 08n09 (April 10, 2006): 1950–61. http://dx.doi.org/10.1142/s0217751x06032897.

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One of the most striking astrophysical phenomena today is the existence of cosmic ray particles with energies in excess of 1020 eV. While their presence has been confirmed by a number of experiments, it is not clear where and how these particles are accelerated to these energies and how they travel astronomical distances without substantial energy loss. We are entering an exciting new era in cosmic ray physics, with instruments now producing data of unprecedented quality and quantity to tackle the many open questions. This paper reviews the current experimental status of cosmic ray physics and summarizes recent results on the energy spectrum and arrival directions of ultra-high-energy cosmic rays.
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Palladino, Andrea, Maurizio Spurio, and Francesco Vissani. "Neutrino Telescopes and High-Energy Cosmic Neutrinos." Universe 6, no. 2 (February 10, 2020): 30. http://dx.doi.org/10.3390/universe6020030.

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In this review paper, we present the main aspects of high-energy cosmic neutrino astrophysics. We begin by describing the generic expectations for cosmic neutrinos, including the effects of propagation from their sources to the detectors. Then we introduce the operating principles of current neutrino telescopes, and examine the main features (topologies) of the observable events. After a discussion of the main background processes, due to the concomitant presence of secondary particles produced in the terrestrial atmosphere by cosmic rays, we summarize the current status of the observations with astrophysical relevance that have been greatly contributed by IceCube detector. Then, we examine various interpretations of these findings, trying to assess the best candidate sources of cosmic neutrinos. We conclude with a brief perspective on how the field could evolve within a few years.
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STANEV, TODOR. "ULTRA HIGH ENERGY COSMIC RAYS: ORIGIN AND PROPAGATION." Modern Physics Letters A 25, no. 18 (June 14, 2010): 1467–81. http://dx.doi.org/10.1142/s0217732310033530.

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We introduce the highest energy cosmic rays and briefly review the powerful astrophysical objects where they could be accelerated. We then introduce the interactions of different cosmic ray particles with the photon fields of the Universe and the formation of the cosmic ray spectra observed at Earth. The last topic is the production of secondary gamma rays and neutrinos in the interactions of the ultrahigh energy cosmic rays.
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Blandford, R. D. "The Phenomena of High Energy Astrophysics." Symposium - International Astronomical Union 214 (2003): 3–20. http://dx.doi.org/10.1017/s0074180900194124.

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A brief summary of some highlights in the study of high energy astrophysical sources over the past decade is presented. It is argued that the great progress that has been made derives largely from the application of new technology to observation throughout all of the electromagnetic and other spectra and that, on this basis, the next decade should be even more exciting. However, it is imperative to observe cosmic sources throughout these spectra in order to obtain a full understanding of their properties. In addition, it is necessary to learn the universal laws that govern the macroscopic and the microscopic behavior of cosmic plasma over a great range of physical conditions by combining observations of different classes of source. These two injunctions are illustrated by discussions of cosmology, hot gas, supernova remnants and explosions, neutron stars, black holes and ultrarelativistic outflows. New interpreations of the acceleration of Galactic cosmic rays, the cooling of hot gas in rich clusters and the nature of ultrarelativistic outflows are outlined. The new frontiers of VHE γ-ray astronomy, low frequency radio astronomy, neutrino astronomy, UHE cosmic ray physics and gravitational wave astronomy are especially promising.
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Okuda, Haruyuki, Guenther Hasinger, Ganesan Srinivasan, Monique D. Arnaud, Sidney A. Bludman, João Braga, Noah Brosch, et al. "DIVISION XI: SPACE & HIGH-ENERGY ASTROPHYSICS." Proceedings of the International Astronomical Union 3, T26B (December 2007): 205–6. http://dx.doi.org/10.1017/s1743921308024125.

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Division XI connects astronomers using space techniques or particle detectors for an extremely large range of investigations, from in-situ studies of bodies in the solar system to orbiting observatories studying the Universe in wavelenghts ranging from radio waves to γ-rays, to underground detectors for cosmic neutrino radiation.
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Hasinger, Günther, Christine Jones, Haruyuki Okuda, João Braga, Noah Brosch, Thijs de Graauw, Leonid I. Gurvits, et al. "DIVISION XI: SPACE & HIGH-ENERGY ASTROPHYSICS." Proceedings of the International Astronomical Union 4, T27A (December 2008): 347–55. http://dx.doi.org/10.1017/s1743921308025830.

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Division XI connects astronomers using space techniques or particle detectors for an extremely large range of investigations, from in-situ studies of bodies in the solar system to orbiting observatories studying the Universe in wavelengths ranging from radio waves to γ-rays, to underground detectors for cosmic neutrino radiation.
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DE RÚJULA, A. "A UNIFIED MODEL OF HIGH-ENERGY ASTROPHYSICAL PHENOMENA." International Journal of Modern Physics A 20, no. 29 (November 20, 2005): 6562–83. http://dx.doi.org/10.1142/s0217751x05029617.

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I outline a unified model of high-energy astrophysics, in which the gamma background radiation, cluster "cooling flows", gamma-ray bursts, X-ray flashes and cosmic-ray electrons and nuclei of all energies — share a common origin. The mechanism underlying these phenomena is the emission of relativistic "cannonballs" by ordinary supernovae, analogous to the observed ejection of plasmoids by quasars and microquasars. I concentrate on Cosmic Rays: the longest-lasting conundrum in astrophysics. The distribution of Cosmic Rays in the Galaxy, their total "luminosity", the broken power-law spectra with their observed slopes, the position of the knee(s) and ankle(s), and the alleged variations of composition with energy are all explained in terms of simple and "standard" physics. The model is only lacking a satisfactory theoretical understanding of the "cannon" that emits the cannonballs in catastrophic episodes of accretion onto a compact object.
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Dissertations / Theses on the topic "High Energy Astrophysics; Cosmic Rays"

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Lee, Anthony A. "Application of Monte Carlo methods to some problems in high energy astrophysics /." Title page, contents and abstract only, 1993. http://web4.library.adelaide.edu.au/theses/09PH/09phl4768.pdf.

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Chadwick, Mary Paula. "Very high energy cosmic gamma rays from radio and X-ray pulsars." Thesis, Durham University, 1987. http://etheses.dur.ac.uk/6720/.

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This thesis is concerned with the detection of very high energy cosmic gamma-rays from isolated pulsars and X-ray binary sources using the atmospheric Cerenkov technique. A general introduction to gamma ray detection techniques is followed by adscription of the properties of atmospheric Cerenkov radiation and a discussion of the principles of the atmospheric Cerenkov technique. The Mark I and Mark II gamma-ray telescopes operated in Dugway, Utah by the University of Durham between 1981 and 1984 are briefly described. There follows a discussion of the results from observations at many different wavelengths of Cygnus X-3. This object was observed by the Durham group between 1981 and 1983 in Dugway Utah and also in Durham during autumn 1985. The detection in the Dugway data of the 4.8 hr X-ray period and the possible detection of a19.2 day intensity variation are considered. The discovery of a 12.59 ms pulsar in data taken on Cygnus X-3 in 1983 is described. Evidence is presented which suggests this periodicity is also present at a weaker level in earlier data and also in the data taken in Durham in 1985.Results from observations of PSR1937+21 , PSR1953+29and six radio pulsars , are presented. The design and construction of the Mark III telescope, now operating in Narrabri , N.S.W. , is described in detail. Preliminary results from observations with the Mark III telescope of three objects, LMC X-4, the Vela pulsar and CentaurusX-3, are presented, with particular reference to periodicities inherent in the sources. An observation of the supernova in the Large Magellanic Cloud is discussed. A brief discussion of the mechanisms by which V.H.E. gamma-rays may be produced in isolated pulsars and X-ray binary pulsars is given, followed by a description of the future prospects for the Mark III and Mark IV telescopes.
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Taylor, Andrew Martin. "The propagation of ultra high energy cosmic rays." Thesis, University of Oxford, 2007. http://ora.ox.ac.uk/objects/uuid:63572ebe-fb32-41b6-8b91-a7294db135a6.

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This thesis presents theoretical work on the propagation of ultra high energy cosmic rays, from their source to Earth. The different energy loss processes, resulting from cosmic ray interactions with the radiation fields, are addressed. The subsequent uncertainties in the energy loss rates and the effect produced on the arriving cosmic ray spectrum are highlighted. The question of the composition of ultra high energy cosmic rays remains unresolved, with the range of possibilities leading to quite different results in both the secondary fluxes of particles produced through cosmic ray energy loss interactions en route, and the arriving cosmic ray spectra at Earth. A large range of nuclear species are considered in this work, spanning the range of physically motivated nuclear types ejected from the cosmic ray source. The treatment of cosmic ray propagation is usually handled through Monte Carlo simulations due to the stochastic nature of some of the particle physics processes relevant. In this work, an analytic treatment for cosmic ray nuclei propagation is developed. The development of this method providing a deeper understanding of the main components relevant to cosmic ray nuclei propagation, and through its application, a clear insight into the contributing particle physics aspects of the Monte Carlo simulation. A flux of secondary neutrinos, produced as a consequence of cosmic ray energy loss through pion production during propagation, is also expected to be observed at Earth. This spectrum, however, is dependent on several loosely constrained factors such as the radiation field in the infrared region and cosmic ray composition. The range of possible neutrino fluxes obtainable with such uncertainties are discussed in this work. High energy cosmic ray interactions with the radiation fields present within the source may also occur, leading to cosmic ray energy loss before the cosmic ray has even managed to escape. The secondary spectra produced are investigated through the consideration of three candidate sources. A relationship between the degree of photo-disintegration in the source region and the neutrino flux produced through p γ interactions is found.
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Brandt, Theresa J. "On High Energy Cosmic Rays from the CREAM Instrument." The Ohio State University, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=osu1259540765.

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Szabo, Anthony Paul. "High energy emissions for astrophysical objects." Title page, contents and abstract only, 1992. http://web4.library.adelaide.edu.au/theses/09PH/09phs996.pdf.

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Gabici, Stefano. "Gamma ray astronomy and the origin of galactic cosmic rays." Habilitation à diriger des recherches, Université Paris-Diderot - Paris VII, 2011. http://tel.archives-ouvertes.fr/tel-00719791.

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Diffusive shock acceleration operating at expanding supernova remnant shells is by far the most popular model for the origin of galactic cosmic rays. Despite the general consensus received by the model, an unambiguous and conclusive proof of the supernova remnant hypothesis is still missing. In this context, the recent developments in gamma ray astronomy provide us with precious insights into the problem of the origin of galactic cosmic rays, since production of gamma rays is expected both during the acceleration of cosmic rays at supernova remnant shocks and during their subsequent propagation in the interstellar medium. In particular, the recent detection of a number of supernova remnants at TeV energies nicely fits with the model, but it still does not constitute a conclusive proof of it, mainly due to the difficulty of disentangling the hadronic and leptonic contributions to the observed gamma ray emission. The main goal of my research is to search for an unambiguous and conclusive observational test for proving (or disproving) the idea that supernova remnants are the sources of galactic cosmic rays with energies up to (at least) the cosmic ray knee. Our present comprehension of the mechanisms of particle acceleration at shocks and of the propagation of cosmic rays in turbulent magnetic fields encourages beliefs that such a conclusive test might come from future observations of supernova remnants and of the Galaxy in the almost unexplored domain of multi-TeV gamma rays.
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MacRae, John Hamish Kenneth. "The detection of very high energy cosmic gamma rays using the atmospheric Cerenkov technique." Thesis, Durham University, 1985. http://etheses.dur.ac.uk/7854/.

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This thesis is concerned with the detection of very high energy cosmic gamma rays using the atmospheric Cerenkov technique. A general introduction to gamma ray detection techniques is followed by a detailed discussion of the principles of the atmospheric Cerenkov technique and the history of its use prior to this work. The design and operation of the University of Durham facility in Dugway, Utah is described in depth. Monte Carlo computer simulations have been developed to assist in both the understanding of the equipment and the analysis of the results for the Durham facility. The variation of the response of the array with zenith angle and detector threshold has been investigated and the aperture function of a single telescope calculated. The latter has been found to be a complicated function of both zenith angle and detector threshold. Computer simulations have also been developed to aid in the design of a camera to record two-dimensional Cerenkov light images from small extensive air showers, and to provide a means of testing analysis routines; these are discussed. The camera is located at the F.L. Whipple Observatory in Arizona. The techniques employed in the analysis of data recorded by the Dugway facility are discussed, and a computer package developed to aid in the routine aspects of the analysis is described. Results of observations from two sources, Cygnus X-3 and PSR0531, are presented, with particular reference to periodicities inherent in the sources and to bursts of gamma ray emission. The discussion of the results includes a review of the various models which have been proposed for Cygnus X-3.
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Morris, Chad Michael. "Detection Techniques of Radio Emission from Ultra High Energy Cosmic Rays." The Ohio State University, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=osu1254506832.

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Pinzke, Anders. "Gamma-Ray Emission from Galaxy Clusters : DARK MATTER AND COSMIC-RAYS." Doctoral thesis, Stockholms universitet, Fysikum, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-42453.

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The quest for the first detection of a galaxy cluster in the high energy gamma-ray regime is ongoing, and even though clusters are observed in several other wave-bands, there is still no firm detection in gamma-rays. To complement the observational efforts we estimate the gamma-ray contributions from both annihilating dark matter and cosmic-ray (CR) proton as well as CR electron induced emission. Using high-resolution simulations of galaxy clusters, we find a universal concave shaped CR proton spectrum independent of the simulated galaxy cluster. Specifically, the gamma-ray spectra from decaying neutral pions, which are produced by CR protons, dominate the cluster emission. Furthermore, based on our derived flux and luminosity functions, we identify the galaxy clusters with the brightest galaxy clusters in gamma-rays. While this emission is challenging to detect using the Fermi satellite, major observations with Cherenkov telescopes in the near future may put important constraints on the CR physics in clusters. To extend these predictions, we use a dark matter model that fits the recent electron and positron data from Fermi, PAMELA, and H.E.S.S. with remarkable precision, and make predictions about the expected gamma-ray flux from nearby clusters. In order to remain consistent with the EGRET upper limit on the gamma-ray emission from Virgo, we constrain the minimum mass of substructures for cold dark matter halos. In addition, we find comparable levels of gamma-ray emission from CR interactions and dark matter annihilations without Sommerfeld enhancement.
At the time of the doctoral defense, the following papers were unpublished and had a status as follows: Paper 2: Accepted.
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Burton, Ross E. "Upper Limits on the Ultra-High Energy Cosmic Ray Flux from Unresolved Sources." Case Western Reserve University School of Graduate Studies / OhioLINK, 2012. http://rave.ohiolink.edu/etdc/view?acc_num=case1323452264.

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Books on the topic "High Energy Astrophysics; Cosmic Rays"

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Clay, Roger. Cosmic bullets: High energy particles in astrophysics. Reading, Mass: Addison-Wesley, 1998.

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1959-, Dawson Bruce, ed. Cosmic bullets: High energy particles in astrophysics. St Leonards, NSW, Australia: Allen & Unwin, 1997.

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Clay, Roger. Cosmic bullets: High energy particles in astrophysics. Reading, Mass: Addison-Wesley, 1997.

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Uryson, Anna. Ultra high energy cosmic rays: A new tool for astrophysics research. Hauppauge, N.Y: Nova Science Publishers, 2009.

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Uryson, Anna. Ultra high energy cosmic rays: A new tool for astrophysics research. New York: Nova Science Publishers, 2010.

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High energy astrophysics. 2nd ed. Cambridge [England]: Cambridge University Press, 1994.

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Lemoine, Martin, and Günter Sigl, eds. Physics and Astrophysics of Ultra-High-Energy Cosmic Rays. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/3-540-45615-5.

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Schröder, Frank G. Instruments and Methods for the Radio Detection of High Energy Cosmic Rays. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012.

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European Cosmic Ray Symposium (15th 1996 Perpignan, France). Cosmic rays 97: Solar, heliospheric, astrophysical, and high energy aspects : proceedings of the 15th European Cosmic Ray Symposium : Perpignan, France, 26-30 August 1996. [Amsterdam]: North-Holland, 1998.

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European, Cosmic Ray Symposium (14th 1994 Balatonfüred Hungary). Cosmic rays 94: Solar, heliospheric, astrophysical and high-energy aspects : proceedings of the 14th European Cosmic Ray Symposium, Balatonfüred, Hungary, 28 August - 3 September 1994. Amsterdam, The Netherlands: North-Holland, 1995.

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Book chapters on the topic "High Energy Astrophysics; Cosmic Rays"

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Horvath, Jorge Ernesto. "Cosmic Rays." In High-Energy Astrophysics, 237–55. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-92159-0_12.

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Spurio, Maurizio. "Ultra High Energy Cosmic Rays." In Astronomy and Astrophysics Library, 203–41. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-08051-2_7.

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Wdowczyk, J. "Anisotropies of High Energy Cosmic Rays." In Cosmic Radiation in Contemporary Astrophysics, 149–59. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-5488-5_10.

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Yodh, Gaurang B. "Ultra High Energy Astronomy." In Cosmic Gamma Rays, Neutrinos, and Related Astrophysics, 183–210. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0921-2_13.

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Silberberg, R., C. H. Tsao, and M. M. Shapiro. "Source Composition of Cosmic-Rays and Models of Origin." In Currents in High-Energy Astrophysics, 87–101. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0253-7_8.

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Swordy, Simon. "Cosmic Ray Elemental Abundances at High Energy." In Cosmic Gamma Rays, Neutrinos, and Related Astrophysics, 481–89. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0921-2_34.

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Berezinsky, Venya. "Course 5: Ultra High Energy Cosmic Rays." In Accretion discs, jets and high energy phenomena in astrophysics, 233–49. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39932-2_5.

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Baring, Matthew G. "Cosmic Gamma-Ray Bursts." In Currents in High-Energy Astrophysics, 21–30. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0253-7_2.

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Courvoisier, Thierry J. L. "The Diffuse X-Ray Background and Other Cosmic Backgrounds." In High Energy Astrophysics, 321–27. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-30970-0_21.

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Spurio, Maurizio. "The Extragalactic Sources and Ultra High Energy Cosmic Rays." In Astronomy and Astrophysics Library, 225–67. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-96854-4_7.

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Conference papers on the topic "High Energy Astrophysics; Cosmic Rays"

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Engel, Ralph, Mariana Orellana, Matías M. Reynoso, Gabriela S. Vila, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, and Oscar Saavedra. "High-energy cosmic ray interactions." In COSMIC RAYS AND ASTROPHYSICS: Proceedings of the 3rd School on Cosmic Rays and Astrophysics. AIP, 2009. http://dx.doi.org/10.1063/1.3141378.

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Gaisser, T. K. "Origin of high energy galactic cosmic rays." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39149.

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Meszaros, Peter. "High-energy astrophysics, (neutrinos, cosmic rays, GRBs)." In XIII Nuclei in the Cosmos. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.204.0188.

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Kalli, Sihem, Martin Lemoine, Kumiko Kotera, N. Mebarki, and J. Mimouni. "Ultra High Energy Cosmic Rays Anisotropies Signatures." In THE THIRD ALGERIAN WORKSHOP ON ASTRONOMY AND ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3518323.

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Matthiae, Giorgio, Da-Shin Lee, Wolung Lee, and She-Sheng Xue. "Results from the Auger Observatory on high-energy cosmic rays." In RELATIVISTIC ASTROPHYSICS: 5th Sino-Italian Workshop on Relativistic Astrophysics. AIP, 2008. http://dx.doi.org/10.1063/1.3012270.

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Golup, Geraldina, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, and Oscar Saavedra. "Source position and magnetic field reconstruction from ultra-high energy cosmic rays arrival directions." In COSMIC RAYS AND ASTROPHYSICS: Proceedings of the 3rd School on Cosmic Rays and Astrophysics. AIP, 2009. http://dx.doi.org/10.1063/1.3141363.

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Taylor, Andrew, Alexandra De Castro, Edith Castillo-Ruiz, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, and Oscar Saavedra. "Ultra High Energy Cosmic Ray, Neutrino, and Photon Propagation and the Multi-Messenger Approach." In COSMIC RAYS AND ASTROPHYSICS: Proceedings of the 3rd School on Cosmic Rays and Astrophysics. AIP, 2009. http://dx.doi.org/10.1063/1.3141380.

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Olum, Ken D. "Ultra-high-energy cosmic rays from relic topological defects." In RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP, 2001. http://dx.doi.org/10.1063/1.1419669.

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BLASI, PASQUALE. "THEORETICAL ASPECTS OF ULTRA HIGH ENERGY COSMIC RAYS." In Proceedings of the XXI Symposium on Relativistic Astrophysics. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812704009_0035.

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Navarra, G. "Experimental results on high energy cosmic rays." In The 3rd international symposium on nuclear astrophysics: Nuclei in the Cosmos III. AIP, 1995. http://dx.doi.org/10.1063/1.47338.

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Reports on the topic "High Energy Astrophysics; Cosmic Rays"

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Tajima, T., and Y. Takahashi. Laboratory laser acceleration and high energy astrophysics: {gamma}-ray bursts and cosmic rays. Office of Scientific and Technical Information (OSTI), August 1998. http://dx.doi.org/10.2172/674811.

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Fowler, T., S. Colgate, and H. Li. On the Origin of Ultra High Energy Cosmic Rays. Office of Scientific and Technical Information (OSTI), July 2009. http://dx.doi.org/10.2172/963520.

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Fowler, T., S. Colgate, H. Li, R. Bulmer, and J. Pino. On the Origin of Ultra High Energy Cosmic Rays II. Office of Scientific and Technical Information (OSTI), March 2011. http://dx.doi.org/10.2172/1021558.

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Chen, Pisin. Plasma Wake Field Acceleration for Ultra High-Energy Cosmic Rays. Office of Scientific and Technical Information (OSTI), July 2002. http://dx.doi.org/10.2172/799975.

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Murase, Kohta, Kunihito Ioka, Shigehiro Nagataki, and Takashi Nakamura. High Energy Neutrinos and Cosmic-Rays From Low-Luminosity Gamma-Ray Bursts? Office of Scientific and Technical Information (OSTI), July 2006. http://dx.doi.org/10.2172/886791.

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Collica, Laura. Mass composition studies of Ultra High Energy cosmic rays through the measurement of the Muon Production Depths at the Pierre Auger Observatory. Office of Scientific and Technical Information (OSTI), January 2014. http://dx.doi.org/10.2172/1249492.

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Soleiman, M. H. M., S. S. Abdel-Aziz, and A. Abdelfattah Omar. Identification of nuclear mass range of primary event from the observation of shower in ultra-high energetic cosmic rays at energy ~ 106 GeV. MTPR Journal, September 2019. http://dx.doi.org/10.19138/mtpr/(19)45-49.

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You might also be interested in the extended bibliographies on the topic 'High Energy Astrophysics; Cosmic Rays' for particular source types:
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